Dear colleagues, New variable star discovery by the MISAO Project (MisV0915). MisV0915 R.A. 18h56m45s.43 Decl. +13o49'40".9 (2000.0) Mag. 13.0C-15.7C Type M? = IRAS 18544+1345 R.A.=18 56 45.10 Decl.=+13 49 33.8 (71 x 12", p.a.=80) flux(12)=0.35 flux(25)=<0.29 flux(60)=<0.43 flux(100)=<18.14 http://vsnet.aerith.net/misao/data/MisV/MisV0915.gif MisV0915 19990707.66400 134C Mis image="KenIchi Kadota" MisV0915 19990707.66444 134C Mis image="KenIchi Kadota" MisV0915 19990923.47453 130C Mis image="KenIchi Kadota" MisV0915 19990923.47497 130C Mis image="KenIchi Kadota" MisV0915 20000508.61000 157C Mis image="Nobuo Ohkura" MisV0915 20000508.61185 156C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV0915. It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Ohkura comparing with images taken by Kadota, then confirmed by Yoshida. The magnitude are measured automatically by the PIXY system. Image observers' names are noted after "Mis". Please see the URL below for the MISAO Project and the PIXY system. http://vsnet.aerith.net/misao/ -- Seiichi Yoshida comet@aerith.net http://vsnet.aerith.net/